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We study cosmological models with interaction between dark energy (DE) and dark matter (DM). For the interaction term Q in cosmic evolution equations, there is a model-independent degeneracy-breaking (D-B) point when $$Q_{1}$$Q1 (a part of Q) equals to zero, where the interaction can be probed without degeneracy between the constant DE equation of state (EoS).

The model-independent degeneracy-breaking point in cosmological models with interacting Dark Energy and Dark Matter